Forecasting F(Q) cosmology with $\Lambda$CDM background using standard sirens

Understand

Forecast constraints for a Symmetric Teleparallel Gravity model with a $\Lambda$CDM background are made using forthcoming ground and space based gravitational waves observatories.

• A Bayesian analysis resorting to generated mock catalogs shows that LIGO is not expected to be able to distinguish this model from $\Lambda$CDM, while both LISA and the ET will, with the ET outperforming LISA.
• We also show that low redshift events are favored in order to improve the quality of the constrains.